Planned stereo pairs have suitable stereo convergence angles and illumination by design.
In addition to planned stereo pairs, the Pairendipity software can identify overlapping
HiRISE images that are serendipitously suitable for stereo processing and find stereo
pairs within the CTX dataset.
Planned HiRISE stereo pairs are listed in the “Stereo Pair List (CSV)” link below.
Since this list is based on produced stereo anaglyphs it also contains a few serendipitous
pairs that underwent special processing. Most serendipitous HiRISE stereo pairs are listed
in the “Pairendipity Stereo” link, while CTX stereo pairs are listed
in “Pairendipity CTX Stereo”.
Images taken close together in time minimize illumination and frost differences and are
especially useful (see the Delta-Days column in the Pairendipity files or difference
the orbit numbers in the image IDs in the Stereo Pair List file). Stereo pairs
with both images planned within the same 14-day (168-orbit) operations cycle are known as SPORCs.
| Dune Interaction with Residual Polar Ice: ESP_089075_2590 ESP_088983_2590 (Interval in Earth days: 8) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | 79.02 | 81.5 | 19.5 | 4.815 | 58.2 | 58.4 |
| Valleys in Terra Cimmeria: ESP_088890_1800 ESP_089391_1800 (Interval in Earth days: 39) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | 0.027 | 123. | -6.7 | 12.85 | 56.6 | 55.2 |
| Eruptive Center in Arcadia Planitia: ESP_089164_2265 ESP_089230_2265 (Interval in Earth days: 5) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | 46.26 | 195. | 8.34 | -6.10 | 46.8 | 48.6 |
| Crater Deposits: ESP_088867_2175 ESP_079927_2175 (Interval in Earth days: 696) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | 37.05 | 28.6 | -18. | -8.45 | 46.7 | 46.2 |
| The Persistence of Dust: ESP_087831_1860 ESP_088042_1860 (Interval in Earth days: 16) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | 5.837 | 237. | 10.3 | -7.81 | 49.9 | 52.0 |
| Stacked!: ESP_089198_1885 ESP_089343_1885 (Interval in Earth days: 11) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | 8.276 | 352. | 4.96 | 19.07 | 52.2 | 51.2 |
| Terrain Southwest of Jovis Tholus: ESP_088411_1960 ESP_088978_1960 (Interval in Earth days: 44) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | 15.96 | 239. | 5.80 | -9.01 | 47.5 | 49.9 |
| Planned ExoMars Landing Site in Oxia Planum: ESP_088658_1990 ESP_088724_1990 (Interval in Earth days: 5) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | 19.01 | 335. | 2.38 | -19.7 | 47.3 | 49.3 |
| Alluvial Fans and Terraced Scarps in Kasei Valles: ESP_088541_2025 ESP_088330_2025 (Interval in Earth days: 16) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | 22.38 | 291. | -19. | -6.13 | 47.7 | 46.0 |
| Dune Monitoring near Utopia Rupes: ESP_088746_2270 ESP_089036_2270 (Interval in Earth days: 23) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | 46.72 | 88.9 | -3.2 | 12.36 | 45.4 | 45.6 |
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